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Acknowledgments
This investigation was undertaken at the suggestion of William C. Martin,
who realized that the hollow-cathode spectrum of platinum would probably have
to be newly measured in order for the Goddard High Resolution Spectrograph to
meet its design goals. His encouragement and suggestions throughout the work
are gratefully acknowledged. Our photoelectric scans of the Pt/Ne lamp on the
10.7 m spectrograph owe much of their success to suggestions of Richard
Deslattes regarding photon counting techniques. We thank him for lending us
his expertise as well as much of the equipment required to carry out the
experiment. Many of the impurity lines in our list were identified by Jean
Blaise. We thank him and Jean-Francois Wyart for making available their new
classifications in Pt I and
Pt II for inclusion in the atlas. This work was
supported in part by the National Aeronautics and Space Administration.